README web version of /home/usg/OPS/MTS/readme_xml/readme_79505500
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our on-going GMRT survey (300 hrs of telescope time) for 21-cm absorbers
at
1.10 < z < 1.45 has uncovered 5 new systems out of 16 candidates searched
till now.
One of the systems, at z = 1.36086 towards J2340-0037, shows a very narrow ( 1 km/s)
and strong 21-cm absorption line. A public KECK spectrum with low SNR=15 and resolution
R=35000 shows a well detached SiII component at the redshift of the 21-cm line.
By comparing the position of the 21cm absorption to that of the corresponding absorption
in the UV, it is possible to constrain the variation of the constant x = alpha^2
G_p\mu.
The existing KECK data itself provides already a good constraint from a single system
at this redshift Delta x/x = (1.27+_2.96)x10^{-6}.
The UVES data of much better SNR and resolution will improve the constraint
by a factor of 3 and provide an independent discriminator for the ongoing
controversy about the variation of alpha.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:20 2009
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